Source code for pycbc.waveform.waveform_modes

# Copyright (C) 2020  Collin Capano, Alex Nitz
# This program is free software; you can redistribute it and/or modify it
# under the terms of the GNU General Public License as published by the
# Free Software Foundation; either version 3 of the License, or (at your
# option) any later version.
#
# This program is distributed in the hope that it will be useful, but
# WITHOUT ANY WARRANTY; without even the implied warranty of
# MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE.  See the GNU General
# Public License for more details.
#
# You should have received a copy of the GNU General Public License along
# with this program; if not, write to the Free Software Foundation, Inc.,
# 51 Franklin Street, Fifth Floor, Boston, MA  02110-1301, USA.

"""Provides functions and utilities for generating waveforms mode-by-mode.
"""

from string import Formatter
import lal

from pycbc import libutils, pnutils
from pycbc.types import (TimeSeries, FrequencySeries)
from .waveform import (props, _check_lal_pars, check_args)
from . import parameters

lalsimulation = libutils.import_optional('lalsimulation')

def _formatdocstr(docstr):
    """Utility for formatting docstrings with parameter information.
    """
    return docstr.format(
        **{_p[1]: getattr(parameters, _p[1]).docstr(
            prefix="    ", include_label=False).lstrip(' ')
           for _p in Formatter().parse(docstr) if _p[1] is not None
           })


def _formatdocstrlist(docstr, paramlist, skip_params=None):
    """Utility for formatting docstrings with parameter information.
    """
    if skip_params is None:
        skip_params = []
    pl = '\n'.join([_p.docstr(prefix="    ", include_label=False)
                    for _p in paramlist if _p not in skip_params]).lstrip(' ')
    return docstr.format(params=pl)


[docs]def sum_modes(hlms, inclination, phi): """Applies spherical harmonics and sums modes to produce a plus and cross polarization. Parameters ---------- hlms : dict Dictionary of ``(l, m)`` -> complex ``hlm``. The ``hlm`` may be a complex number or array, or complex ``TimeSeries``. All modes in the dictionary will be summed. inclination : float The inclination to use. phi : float The phase to use. Returns ------- complex float or array The plus and cross polarization as a complex number. The real part gives the plus, the negative imaginary part the cross. """ out = None for mode in hlms: l, m = mode hlm = hlms[l, m] ylm = lal.SpinWeightedSphericalHarmonic(inclination, phi, -2, l, m) if out is None: out = ylm * hlm else: out += ylm * hlm return out
[docs]def default_modes(approximant): """Returns the default modes for the given approximant. """ # FIXME: this should be replaced to a call to a lalsimulation function, # whenever that's added if approximant in ['IMRPhenomXPHM', 'IMRPhenomXHM']: # according to arXiv:2004.06503 ma = [(2, 2), (2, 1), (3, 3), (3, 2), (4, 4)] # add the -m modes ma += [(l, -m) for l, m in ma] elif approximant in ['IMRPhenomPv3HM', 'IMRPhenomHM']: # according to arXiv:1911.06050 ma = [(2, 2), (2, 1), (3, 3), (3, 2), (4, 4), (4, 3)] # add the -m modes ma += [(l, -m) for l, m in ma] elif approximant.startswith('NRSur7dq4'): # according to arXiv:1905.09300 ma = [(l, m) for l in [2, 3, 4] for m in range(-l, l+1)] elif approximant.startswith('NRHybSur3dq8'): # according to arXiv:1812.07865 ma = [(2, 0), (2, 1), (2, 2), (3, 0), (3, 1), (3, 2), (3, 3), (4, 2), (4, 3), (4, 4), (5, 5)] else: raise ValueError("I don't know what the default modes are for " "approximant {}, sorry!".format(approximant)) return ma
[docs]def get_glm(l, m, theta): r"""The maginitude of the :math:`{}_{-2}Y_{\ell m}`. The spin-weighted spherical harmonics can be written as :math:`{}_{-2}Y_{\ell m}(\theta, \phi) = g_{\ell m}(\theta)e^{i m \phi}`. This returns the `g_{\ell m}(\theta)` part. Note that this is real. Parameters ---------- l : int The :math:`\ell` index of the spherical harmonic. m : int The :math:`m` index of the spherical harmonic. theta : float The polar angle (in radians). Returns ------- float : The amplitude of the harmonic at the given polar angle. """ return lal.SpinWeightedSphericalHarmonic(theta, 0., -2, l, m).real
[docs]def get_nrsur_modes(**params): """Generates NRSurrogate waveform mode-by-mode. All waveform parameters should be provided as keyword arguments. Recognized parameters are listed below. Unrecognized arguments are ignored. Parameters ---------- template: object An object that has attached properties. This can be used to substitute for keyword arguments. A common example would be a row in an xml table. approximant : str The approximant to generate. Must be one of the ``NRSur*`` models. {delta_t} {mass1} {mass2} {spin1x} {spin1y} {spin1z} {spin2x} {spin2y} {spin2z} {f_lower} {f_ref} {distance} {mode_array} Returns ------- dict : Dictionary of ``(l, m)`` -> ``(h_+, -h_x)`` ``TimeSeries``. """ laldict = _check_lal_pars(params) ret = lalsimulation.SimInspiralPrecessingNRSurModes( params['delta_t'], params['mass1']*lal.MSUN_SI, params['mass2']*lal.MSUN_SI, params['spin1x'], params['spin1y'], params['spin1z'], params['spin2x'], params['spin2y'], params['spin2z'], params['f_lower'], params['f_ref'], params['distance']*1e6*lal.PC_SI, laldict, getattr(lalsimulation, params['approximant']) ) hlms = {} while ret: hlm = TimeSeries(ret.mode.data.data, delta_t=ret.mode.deltaT, epoch=ret.mode.epoch) hlms[ret.l, ret.m] = (hlm.real(), hlm.imag()) ret = ret.next return hlms
[docs]def get_nrhybsur_modes(**params): """Generates NRHybSur3dq8 waveform mode-by-mode. All waveform parameters should be provided as keyword arguments. Recognized parameters are listed below. Unrecognized arguments are ignored. Parameters ---------- template: object An object that has attached properties. This can be used to substitute for keyword arguments. A common example would be a row in an xml table. approximant : str The approximant to generate. Must be one of the ``NRHyb*`` models. {delta_t} {mass1} {mass2} {spin1z} {spin2z} {f_lower} {f_ref} {distance} {mode_array} Returns ------- dict : Dictionary of ``(l, m)`` -> ``(h_+, -h_x)`` ``TimeSeries``. """ laldict = _check_lal_pars(params) ret = lalsimulation.SimIMRNRHybSur3dq8Modes( params['delta_t'], params['mass1']*lal.MSUN_SI, params['mass2']*lal.MSUN_SI, params['spin1z'], params['spin2z'], params['f_lower'], params['f_ref'], params['distance']*1e6*lal.PC_SI, laldict ) hlms = {} while ret: hlm = TimeSeries(ret.mode.data.data, delta_t=ret.mode.deltaT, epoch=ret.mode.epoch) hlms[ret.l, ret.m] = (hlm.real(), hlm.imag()) ret = ret.next return hlms
get_nrsur_modes.__doc__ = _formatdocstr(get_nrsur_modes.__doc__) get_nrhybsur_modes.__doc__ = _formatdocstr(get_nrhybsur_modes.__doc__)
[docs]def get_imrphenomxh_modes(**params): """Generates ``IMRPhenomXHM`` waveforms mode-by-mode. """ approx = params['approximant'] if not approx.startswith('IMRPhenomX'): raise ValueError("unsupported approximant") mode_array = params.pop('mode_array', None) if mode_array is None: mode_array = default_modes(approx) if 'f_final' not in params: # setting to 0 will default to ringdown frequency params['f_final'] = 0. hlms = {} for (l, m) in mode_array: params['mode_array'] = [(l, m)] laldict = _check_lal_pars(params) hlm = lalsimulation.SimIMRPhenomXHMGenerateFDOneMode( float(pnutils.solar_mass_to_kg(params['mass1'])), float(pnutils.solar_mass_to_kg(params['mass2'])), float(params['spin1z']), float(params['spin2z']), l, m, pnutils.megaparsecs_to_meters(float(params['distance'])), params['f_lower'], params['f_final'], params['delta_f'], params['coa_phase'], params['f_ref'], laldict) hlm = FrequencySeries(hlm.data.data, delta_f=hlm.deltaF, epoch=hlm.epoch) # Plus, cross strains without Y_lm. # (-1)**(l) factor ALREADY included in FDOneMode hplm = 0.5 * hlm # Plus strain hclm = 0.5j * hlm # Cross strain if m > 0: hclm *= -1 hlms[l, m] = (hplm, hclm) return hlms
_mode_waveform_td = {'NRSur7dq4': get_nrsur_modes, 'NRHybSur3dq8': get_nrhybsur_modes, } _mode_waveform_fd = {'IMRPhenomXHM': get_imrphenomxh_modes, } # 'IMRPhenomXPHM':get_imrphenomhm_modes needs to be implemented # LAL function do not split strain mode by mode
[docs]def fd_waveform_mode_approximants(): """Frequency domain approximants that will return separate modes.""" return sorted(_mode_waveform_fd.keys())
[docs]def td_waveform_mode_approximants(): """Time domain approximants that will return separate modes.""" return sorted(_mode_waveform_td.keys())
[docs]def get_fd_waveform_modes(template=None, **kwargs): r"""Generates frequency domain waveforms, but does not sum over the modes. The returned values are the frequency-domain equivalents of the real and imaginary parts of the complex :math:`\mathfrak{{h}}_{{\ell m}}(t)` time series. In other words, the returned values are equivalent to the Fourier Transform of the two time series returned by :py:func:`get_td_waveform_modes`; see that function for more details. Parameters ---------- template: object An object that has attached properties. This can be used to subsitute for keyword arguments. {params} Returns ------- ulm : dict Dictionary of mode tuples -> fourier transform of the real part of the hlm time series, as a :py:class:`pycbc.types.FrequencySeries`. vlm : dict Dictionary of mode tuples -> fourier transform of the imaginary part of the hlm time series, as a :py:class:`pycbc.types.FrequencySeries`. """ params = props(template, **kwargs) required = parameters.fd_required check_args(params, required) apprx = params['approximant'] if apprx not in _mode_waveform_fd: raise ValueError("I don't support approximant {}, sorry" .format(apprx)) return _mode_waveform_fd[apprx](**params)
get_fd_waveform_modes.__doc__ = _formatdocstrlist( get_fd_waveform_modes.__doc__, parameters.fd_waveform_params, skip_params=['inclination', 'coa_phase'])
[docs]def get_td_waveform_modes(template=None, **kwargs): r"""Generates time domain waveforms, but does not sum over the modes. The returned values are the real and imaginary parts of the complex :math:`\mathfrak{{h}}_{{\ell m}}(t)`. These are defined such that the plus and cross polarizations :math:`h_{{+,\times}}` are: .. math:: h_{{+,\times}}(\theta, \phi; t) = (\Re, -\Im) \sum_{{\ell m}} {{}}_{{-2}}Y_{{\ell m}}(\theta, \phi) \mathfrak{{h}}_{{\ell m}}(t). Parameters ---------- template: object An object that has attached properties. This can be used to subsitute for keyword arguments. {params} Returns ------- ulm : dict Dictionary of mode tuples -> real part of the hlm, as a :py:class:`pycbc.types.TimeSeries`. vlm : dict Dictionary of mode tuples -> imaginary part of the hlm, as a :py:class:`pycbc.types.TimeSeries`. """ params = props(template, **kwargs) required = parameters.td_required check_args(params, required) apprx = params['approximant'] if apprx not in _mode_waveform_td: raise ValueError("I don't support approximant {}, sorry" .format(apprx)) return _mode_waveform_td[apprx](**params)
get_td_waveform_modes.__doc__ = _formatdocstrlist( get_td_waveform_modes.__doc__, parameters.td_waveform_params, skip_params=['inclination', 'coa_phase'])